Results 181 to 190 of about 298,499 (308)
Abstract Short Large‐Amplitude Magnetic Structures (SLAMS) are believed to play important roles in the physics governing the formation of quasi‐parallel shocks. These isolated non‐linear structures, frequently observed in the foreshock, have been suggested to be building blocks for the shock and have been shown to drive shock reformation. In this work,
S. Bergman, T. Karlsson, T. K. Wong Chan
wiley +1 more source
Rotational Influence on the Martian Magnetotail Current Sheet: A Multispecies MHD Study
Abstract The Martian magnetotail current sheet exhibits a dawn‐dusk asymmetry, but the reasons for this shift remain unclear. Although crustal magnetic fields influence this asymmetry, most magnetohydrodynamic (MHD) simulations focus on the subsolar orientation of 180°W, 0°N, which places the strongest crustal fields on the dayside and overlooks ...
Nii‐Boi A. Quartey +4 more
wiley +1 more source
Abstract Electric field instruments function by electrically coupling to the surrounding plasma, resulting in a response function that varies depending on local conditions. This variable coupling can complicate quantitative interpretation of wave measurements, yet is rarely considered.
D. P. Hartley +7 more
wiley +1 more source
Isotropic fluid structures and role of non-metricity on their dynamics governed by an electric charge: A theoretical study. [PDF]
Naseer T +4 more
europepmc +1 more source
Abstract We apply a hybrid model (kinetic ions, fluid electrons) to provide context for MErcury Surface Space ENvironment, GEochemistry, and Ranging (MESSENGER) observations of Disappearing Dayside Magnetosphere (DDM) events at Mercury. Such events have been observed on four occasions and are caused by Coronal Mass Ejections completely removing the ...
Georg Glebe +2 more
wiley +1 more source
Intense Ground Magnetic Perturbations During the 2024 May and October Geomagnetic Storms
Abstract The May and October 2024 geomagnetic storms represent two of the most intense space weather events of Solar Cycle 25. While differing in global intensity, both storms produced extreme ionospheric disturbances, including equatorward auroral expansion to mid‐latitudes and rapid geomagnetic variations (dH/dt $\text{dH}/\text{dt}$).
P. De Michelis +3 more
wiley +1 more source
Classification of LRS Bianchi-I spacetime in context of f(T) gravity via its self-similar symmetry. [PDF]
Sidaoui R +5 more
europepmc +1 more source
Abstract We investigated the quiet‐time temporal variations of the Equatorial Ionization Anomaly (EIA) and underlying plasma fountain observed in the topside ionosphere during the various F‐region equatorial E × B drift events recorded by the Jicamarca Incoherent Scatter Radar and simulated by SAMI3.
Ildiko Horvath, Brian C. Lovell
wiley +1 more source
Determination of the mass distribution of the first stars from the 21-cm signal. [PDF]
Gessey-Jones T +8 more
europepmc +1 more source
Augmenting astrophysical scaling relations with machine learning: Application to reducing the Sunyaev-Zeldovich flux-mass scatter. [PDF]
Wadekar D +9 more
europepmc +1 more source

